Metal content of the circumgalactic medium around star-forming galaxies at z ∼ 2.6 as revealed by the VIMOS Ultra-Deep Survey

Open Access

Fig. 9.

Equivalent width (W₀) for the Lyα emission as a function of the impact parameter (b) obtained from the average (solid red line) and median (dot-dashed blue line) composite spectra. The error bars correspond to 1σ confidence intervals for average or median values based on a bootstrap analysis.

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